Result for 14B30D7FAA1AC5E04F9747644FC565316BF02B00

Query result

Key Value
FileName./usr/lib/x86_64-linux-gnu/cpl/plugins/hawki-1.8.14/hawki_step_basic_calib.la
FileSize1049
MD5D563900CE389F5921EE361FE47B008A3
SHA-114B30D7FAA1AC5E04F9747644FC565316BF02B00
SHA-2568CECD1C19461A0CBA775FE07BE724FC4288ADD7F6C985DFC4E9E9CF7855B47A8
SSDEEP24:SeSh+WJEixxIK+Ahmfvi4yvD2NGDe5/bh:SAWJ9xxIK1hmfKtLcbh
TLSHT1D811F07B83CE9229BAE05AA58BCF7C3EC29D84384A255E1452CBC5EB114B41A1356F73
hashlookup:parent-total1
hashlookup:trust55

Network graph view

Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize195760
MD5AD2C0CE7BFA6DD0C55A03053260B56BB
PackageDescriptionESO data reduction pipeline for HAWK-I This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion1.8.14+dfsg-2
SHA-1086A952CA52A913571A4B157A2FACE4144827EDA
SHA-2562D7C4EE843C799609FC589F29F835C883F9AA2BE52375FA434E627D2452C14C0